How statement and proof provenance work
The first chip identifies the source of the statement or construction; the second identifies the source of its local proof or verification.
- Literature-sourced: the exact statement appears in a cited source; only wording and notation differ.
- AI-adapted: a semantically identical restatement of literature-sourced material, modulo indexing, notation, and boundary cases adopted by the library.
- AI-generated: a genuinely novel statement formulated by AI, with no source for the claim itself.
These labels describe origin, not correctness: citations and verification chips remain separate evidence.
A 2026 weak-curvature F-theory QCD-axion ensemble constraint
Source-reported model-population inference for the paper's selected Tree, Skeleton, and K2 toric-threefold ensembles and its selected weak-curvature Kähler points. The SN1987A limit is an approximate astrophysical inference based on the source's supernova-emission model and one-dimensional simulations. The reported fraction is not a probability over all F-theory vacua or a deduction that F-theory describes nature.
Example
Fallon, Halverson, McAllister, and Marsh study source-selected F-theory models on toric threefold bases with , where is the first Hodge number of the compact Kähler base. The source selects a weak-curvature Kähler point for each constructed model, where weak curvature means that corrections are plausibly negligible, and estimates the QCD-axion mass using its stated effective-field-theory and instanton approximation. Across the Tree, Skeleton, and K2 ensembles, the paper reports that in every populated bin at least of its sampled models have , above its adopted approximate SN1987A limit. The source does not provide precise model counts for each bin, and its percentage is a sample frequency for those selected models and Kähler points, not a probability over all F-theory vacua.
The adopted SN1987A limit is an astrophysical inference: the paper uses axion-nucleon emission and the Raffelt criterion, based on one-dimensional supernova simulations of the observed neutrino burst. This is not a reported experiment measuring an F-theory model. The authors do not stabilize moduli and use a proxy visible sector without a suitable , supersymmetry breaking, or fermion couplings.
Example references
Facts & Assumptions
Given: The paper's finite model ensembles, its selected weak-curvature Kähler points and QCD-axion mass approximation, and its source-specific interpretation of the SN1987A neutrino-burst constraint.
Table I reports 14,627 Tree models with , 16,556 Skeleton models with , and 54 K2 models with . The source does not give precise per-bin counts. Its high- bins therefore contain no Tree models. Fallon et al., Table I and Results
The source adopts the approximate QCD-axion mass limit from its axion-nucleon emissivity and Raffelt-criterion analysis of the SN1987A neutrino burst. The criterion is based on one-dimensional supernova simulations; it is an astrophysical inference, not a measured F-theory quantity. The paper does not independently audit the underlying supernova observations or simulations. Fallon et al., SN1987A and the QCD axion
For each constructed model, the authors select a weak-curvature Kähler point using their stated gauge-coupling and supersymmetry-scale conditions, then estimate with their effective-field-theory procedure and a selected subset of instanton scales. Weak curvature is used to argue that corrections are plausibly negligible; this is a source approximation, not a proved error bound. Fallon et al., Methodology
The Results section and Fig. 3 report that in every populated bin with , at least of the sampled models lie above the adopted threshold. The paper gives no precise model count for each such bin. This is the authors' finite-sample report, not a probability statement for a larger population. Fallon et al., Results and Fig. 3
Compact Kähler and rational Hodge polarization conventions fixes the compact Kähler convention for the source's base.
Compact Kähler Hodge decomposition from elliptic harmonic forms identifies with the bidegree- Hodge summand and the Dolbeault group ; it supplies finite-dimensionality under compact-Kähler and full-AC hypotheses.
Type-IIB axiodilaton and elliptic-fiber dictionary adopts the geometric elliptic-fibration/F-theory dictionary. Its current statement supplies the context used here; this item does not use it as a proof of the reported ensemble frequency.
Verification
The source's Table I gives the maximum Tree value , while the Skeleton and K2 ranges include values above the stated threshold. Thus no populated bin with comes from Tree. The totals in [A1] are whole-ensemble counts and do not determine any individual high- bin count.
By [A3], the calculation uses one selected weak-curvature Kähler point per constructed model and a truncated instanton estimate. Comparing these source estimates with the approximate astrophysical inference [A2] therefore concerns those selected model points under the source's approximation, not all points in moduli space or a direct measurement of the compactification.
The source reports the frequency in [A4]. Together with [A1] and the selection procedure in [A3], its scope is the finite sampled ensembles and selected Kähler points. Since the paper gives no per-bin counts, this item makes no stronger count claim; since the sample is selected and finite, the reported percentage is not a probability over all F-theory vacua. Its comparison remains conditional on the astrophysical inference [A2].
Remarks
The source reports that additional axions could strengthen the supernova constraint, but their effect depends on further model assumptions. It also leaves moduli stabilization, a suitable visible-sector , supersymmetry breaking, and fermion couplings unresolved. None of these omissions is repaired by the reported sample frequency.